An inertial model of the interaction of Ekman layers and planetary islands

dc.contributor.author Pedlosky, Joseph
dc.date.accessioned 2014-02-11T19:54:05Z
dc.date.available 2014-02-11T19:54:05Z
dc.date.issued 2013-07
dc.description Author Posting. © American Meteorological Society, 2013. This article is posted here by permission of American Meteorological Society for personal use, not for redistribution. The definitive version was published in Journal of Physical Oceanography 43 (2013): 1398–1406, doi:10.1175/JPO-D-13-028.1. en_US
dc.description.abstract An adiabatic, inertial, and quasigeostrophic model is used to discuss the interaction of surface Ekman transport with an island. The theory extends the recent work of Spall and Pedlosky to include an analytical and nonlinear model for the interaction. The presence of an island that interrupts a uniform Ekman layer transport raises interesting questions about the resulting circulation. The consequential upwelling around the island can lead to a local intake of fluid from the geostrophic region beneath the Ekman layer or to a more complex flow around the island in which the fluid entering the Ekman layer on one portion of the island's perimeter is replaced by a flow along the island's boundary from a downwelling region located elsewhere on the island. This becomes especially pertinent when the flow is quasigeostrophic and adiabatic. The oncoming geostrophic flow that balances the offshore Ekman flux is largely diverted around the island, and the Ekman flux is fed by a transfer of fluid from the western to the eastern side of the island. As opposed to the linear, dissipative model described earlier, this transfer takes place even in the absence of a topographic skirt around the island. The principal effect of topography in the inertial model is to introduce an asymmetry between the circulation on the northern and southern sides of the island. The quasigeostrophic model allows a simple solution to the model problem with topography and yet the resulting three-dimensional circulation is surprisingly complex with streamlines connecting each side of the island. en_US
dc.description.sponsorship This research was supported in part by NSF Grant OCE Grant 0925061. en_US
dc.format.mimetype application/pdf
dc.identifier.citation Journal of Physical Oceanography 43 (2013): 1398–1406 en_US
dc.identifier.doi 10.1175/JPO-D-13-028.1
dc.identifier.uri https://hdl.handle.net/1912/6437
dc.language.iso en_US en_US
dc.publisher American Meteorological Society en_US
dc.relation.uri https://doi.org/10.1175/JPO-D-13-028.1
dc.subject Baroclinic flows en_US
dc.subject Large-scale motions en_US
dc.subject Nonlinear dynamics en_US
dc.subject Ocean circulation en_US
dc.subject Ocean dynamics en_US
dc.subject Topographic effects en_US
dc.title An inertial model of the interaction of Ekman layers and planetary islands en_US
dc.type Article en_US
dspace.entity.type Publication
relation.isAuthorOfPublication f5dbc523-4176-4180-9ef3-b4f6dbff4163
relation.isAuthorOfPublication.latestForDiscovery f5dbc523-4176-4180-9ef3-b4f6dbff4163
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